MAURO
STEFANON -

INVEST DISTING DE EXCELENCIA CV

Foto de MAURO

Foto de Universidad Andrés Bello

Universidad Andrés Bello

Santiago de Chile, Chile

Publicaciones en colaboración con investigadores/as de Universidad Andrés Bello (5)

2022

MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z ≳ 3* * The spectra presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
Astrophysical Journal, Vol. 938, Núm. 2

2020

An Extremely Massive Quiescent Galaxy at z = 3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models
Astrophysical Journal Letters, Vol. 890, Núm. 1
The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching
Astronomy and Astrophysics, Vol. 638
The Massive Ancient Galaxies at z > 3 NEar-infrared (MAGAZ3NE) Survey: Confirmation of Extremely Rapid Star Formation and Quenching Timescales for Massive Galaxies in the Early Universe*
Astrophysical Journal, Vol. 903, Núm. 1

2019

The Rest-frame H-band Luminosity Function of Red-sequence Galaxies in Clusters at 1.0 < z < 1.3
Astrophysical Journal, Vol. 880, Núm. 2